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Ghosts in metric-affine higher order curvature gravity

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arxiv 1901.08988 v2 pith:AJZN7ZU5 submitted 2019-01-25 gr-qc hep-th

Ghosts in metric-affine higher order curvature gravity

classification gr-qc hep-th
keywords gravitymetric-affinetheoriescurvaturehigherorderadditionalconstraints
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We disprove the widespread belief that higher order curvature theories of gravity in the metric-affine formalism are generally ghost-free. This is clarified by considering a sub-class of theories constructed only with the Ricci tensor and showing that the non-projectively invariant sector propagates ghost-like degrees of freedom. We also explain how these pathologies can be avoided either by imposing a projective symmetry or additional constraints in the gravity sector. Our results put forward that higher order curvature gravity theories generally remain pathological in the metric-affine (and hybrid) formalisms and highlight the key importance of the projective symmetry and/or additional constraints for their physical viability and, by extension, of general metric-affine theories.

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Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Degenerate higher-order scalar-tensor theories in metric-affine gravity

    gr-qc 2025-12 unverdicted novelty 7.0

    A metric-affine version of quadratic DHOST theories is derived and reduced to a one-function family that satisfies degeneracy conditions and light-speed gravitational wave propagation.

  2. Nonrotating and rotating black holes with secondary disformal hair in a ghost-free metric-affine parity-violating scalar-torsion theory

    gr-qc 2026-06 unverdicted novelty 6.0

    Exact Schwarzschild and Kerr geometries in a disformally related frame yield secondary disformal scalar hair on black holes in a projectively invariant scalar-torsion theory.

  3. Naturally Light Distortion

    gr-qc 2026-03 unverdicted novelty 5.0

    A naturally light scalar-like distortion field emerges in generalized gravity and mixes with the Higgs boson.